Äîêóìåíò âçÿò èç êýøà ïîèñêîâîé ìàøèíû. Àäðåñ îðèãèíàëüíîãî äîêóìåíòà : http://www.atnf.csiro.au/people/Ray.Norris/emu/askap/index.htm
Äàòà èçìåíåíèÿ: Fri Apr 8 09:19:57 2016
Äàòà èíäåêñèðîâàíèÿ: Sun Apr 10 17:36:26 2016
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Ïîèñêîâûå ñëîâà: annular solar eclipse
EMU: Evolutionary Map of the Universe
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ASKAP

ASKAP Specifications

Background

ASKAP (Australian Square Kilometre Array Pathfinder) is a new radio-telescope being constructed in Australia. ˆàIt differs from previous radio-telescopes in several important respects, including

  • a phased-array feed which will enable efficient surveys of large areas of the sky,
  • the way in which it will be operated, with users interacting with it primarily through the data archive rather than hands-on operation of the telescope.

Access to the telescope is open to all users, regardless of nationality or institution. Science operations are expected to commence in 2016. Details may be found on http://www.atnf.csiro.au/projects/askap/

Specifications

  • The final system will have 36 dishes, each 12 m diameter
  • Each antenna equipped with a 188 x 2pol FPA mounted at the prime focus
  • System temperature (Tsys) of ~50ˆàK
  • Frequency range 0.7 òÀÓ 1.8 GHz
  • Instantaneous bandwidth 300 MHz
  • At least 30 independent beams giving a total field of view of 30 sq deg over the entire frequency range
  • Maximum baseline 6 km
  • Full cross-correlation of all antennas
  • Correlator located at the ASKAP site, with a high-bandwidth fibre taking correlated data to Perth for archiving and processing.

Configuration

See http://wwwatnf.atnf.csiro.au/projects/askap/config.html

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This page last updated by Ray Norris 7-Nov-2008

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